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ρ0 Photoproduction In Auau Collisions At √s Nn=62.4 Gev Measured With The Star Detector

机译:用星探测器在√sNn = 62.4 Gev的Auau碰撞中产生ρ0的光产生

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摘要

Vector mesons may be photoproduced in relativistic heavy-ion collisions when a virtual photon emitted by one nucleus scatters from the other nucleus, emerging as a vector meson. The STAR Collaboration has previously presented measurements of coherent ρ0 photoproduction at center of mass energies of 130 GeV and 200 GeV in AuAu collisions. Here, we present a measurement of the cross section at 62.4 GeV; we find that the cross section for coherent ρ0 photoproduction with nuclear breakup is 10.5±1.5±1.6 mb at 62.4 GeV. The cross-section ratio between 200 GeV and 62.4 GeV is 4.4±0.6, less than is predicted by most theoretical models. It is, however, proportionally much larger than the previously observed 15%±55% increase between 130 GeV and 200 GeV. © 2012 American Physical Society.
机译:当一个原子核发射的虚拟光子从另一个原子核散射而成为矢量介子时,矢量介子可能在相对论重离子碰撞中被光生。 STAR Collaboration先前已经提出了在AuAu碰撞中在130 GeV和200 GeV质能中心的相干ρ0光产生的测量值。在这里,我们给出了在62.4 GeV处的横截面测量值。我们发现在62.4 GeV时相干ρ0光产生与核破裂的横截面为10.5±1.5±1.6 mb。 200 GeV和62.4 GeV之间的截面比为4.4±0.6,小于大多数理论模型所预测的。但是,它比130 GeV和200 GeV之间的15%±55%的增量成比例地大得多。 ©2012美国物理学会。

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